1972Indian Institute of AstrophysicsRequires access

The Frequency Drift and Time Splitting of Decameter Solar Radio Bursts

Ch. V. Sastry

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Abstract

The frequency drift and time splitting of solar radio bursts are observed \nwith a multi-channel radiometer and a polarimeter at frequencies around 25 \nMHz. It is found that a majority of noise storm bursts have drift rates \nbetween + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency \ndrift are described. The two components of a double burst are found to be \npolarized to the same degree and in the same sense.

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The frequency drift and time splitting of solar radio bursts are observed \nwith a multi-channel radiometer and a polarimeter at frequencies around 25 \nMHz. It is found that a majority of noise storm bursts have drift rates \nbetween + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency \ndrift are described. The two components of a double burst are found to be \npolarized to the same degree and in the same sense.

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Available abstract

The frequency drift and time splitting of solar radio bursts are observed \nwith a multi-channel radiometer and a polarimeter at frequencies around 25 \nMHz. It is found that a majority of noise storm bursts have drift rates \nbetween + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency \ndrift are described. The two components of a double burst are found to be \npolarized to the same degree and in the same sense.

Key concepts: Solar radio, Physics, Astrophysics, Astronomy, Solar physics, Solar flare

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